Compton Electron

2016 ◽  
Author(s):  
M. De Bruin
Keyword(s):  
1978 ◽  
Vol 18 (5) ◽  
pp. 613-616 ◽  
Author(s):  
G. M. Gandel'man ◽  
V. V. Ivanov ◽  
Yu. A. Medvedev ◽  
B. M. Stepanov ◽  
G. V. Fedorovich

Author(s):  
N.A. Guardala ◽  
J.L. Price ◽  
D.J. Land ◽  
D.G. Simons ◽  
D.H. Lee ◽  
...  

1957 ◽  
Vol 105 (2) ◽  
pp. 619-624 ◽  
Author(s):  
J. W. Robson ◽  
E. C. Gregg

2020 ◽  
Vol 6 ◽  
pp. 338
Author(s):  
N. P. Vodinas ◽  
C. W. De Jager ◽  
N. H. Papadakis ◽  
I. Passchier

The longitudinal polarization of the stored electron beam in the AmPS ring will be measured through the laser Compton backscattering technique. With the outlined design the measurement of the expected 70% degree of polarization to a statistical precision of 3% requires less than 60 sec under ideal conditions.


1971 ◽  
Vol 41 ◽  
pp. 58-62 ◽  
Author(s):  
F. Albernhe ◽  
C. Doulade ◽  
I. M. Martin ◽  
R. Talon ◽  
G. Vedrenne

A stilbene scintillator detector allowing gamma-ray spectrometry in the range 0.5–5 MeV is presented. A complete elimination of charged particles is obtained by a plastic scintillator anticoïncidence jacket. Separation of gamma rays from neutrons is made by pulse shape discrimination technique with over 99% efficiency. This detector which has a 4 π field of view has been made as light as possible to avoid perturbation due to secondary production in the apparatus. The correction of the edge effects and the method of conversion from experimental Compton electron spectrum to gamma-ray spectrum are explained.Results from balloon launchings at three latitudes (Kourou Guyana: 10 N, Aire sur l'Adour: 46°N and Oboziersky U.S.S.R.: 62 °N) are briefly presented. The detection possibility with balloons of galactic gamma rays at equatorial latitude is shown. The atmospheric part of the flux at the equator is deduced from the measurements at higher latitudes, (46 °N and 62 °N) where the galactic component is of negligible importance. Assuming a power law spectrum and after correction of the atmospheric absorption we obtain for the galactic spectrum the expression dN/dE = 1.1 × 10−5E−1, 2 photons/cm2 s sr keV. This spectrum agrees with the results of ERS 18 satellite given by Vette et al. showing an excess of flux for energies higher than 1 MeV.


1953 ◽  
Vol 31 (4) ◽  
pp. 592-603 ◽  
Author(s):  
R. M. Pearce ◽  
K. C. Mann

A method of suppression of the Compton electron background present in photoelectron spectra is described. The method employs an anticoincidence element which eliminates Compton electron pulses in the spectrometer detector counter and leaves photoelectron pulses unaffected. The technique has been applied to the photoelectron spectra of Co60, Ta182, and Ra (B + C). Evidence is presented for a previously unreported 1.01 Mev. gamma-ray transition in Ta182. The spectrum of Ra (B + C) is compared with the spectra reported by Ellis and by Latyshev. Some of the new transitions found by Latyshev are confirmed. Other gamma-rays not reported by other workers are presented here.


2014 ◽  
Vol 105 (18) ◽  
pp. 184101 ◽  
Author(s):  
A. Haefner ◽  
D. Gunter ◽  
B. Plimley ◽  
R. Pavlovsky ◽  
K. Vetter

1960 ◽  
Vol 38 (6) ◽  
pp. 720-750 ◽  
Author(s):  
G. E. Lee-Whiting

Improvements in the design of one type of Compton-electron spectrometer for γ-rays are proposed. The design requires a magnetic field of cylindrical symmetry and of slow radial variation, a simply curved radiator, and a system of apertures. Electrons are accepted only if they are ejected from the radiator with small components of momentum in two orthogonal directions perpendicular to the incident γ-ray. Since the magnetic field can also be used to measure the momentum of the selected electrons, the instrument can function as a γ-ray spectrometer. Higher-order aberrations are discussed, and a method of calculating the values of the various spectrometer parameters corresponding to maximum efficiency is given. Calculations of the intrinsic line-width, caused by the motion of the electron within the atom before collision with the photon, are carried out.


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